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Numerical Methods in Quantum Mechanics - Dipartimento di Fisica

Numerical Methods in Quantum Mechanics - Dipartimento di Fisica

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number of possible Slater determ<strong>in</strong>ants a subset of most significant ones. Such<br />

technique, computationally very heavy, is used <strong>in</strong> quantum chemistry to get<br />

high-precision results <strong>in</strong> small molecules. Other, less heavy methods (the socalled<br />

Møller-Plesset, MP, approaches) rely on perturbation theory to yield a<br />

rather good estimate of correlation energy. A completely <strong>di</strong>fferent approach,<br />

which produces equations that are rem<strong>in</strong>iscent of Hartree-Fock equations, is<br />

Density-Functional Theory (DFT), much used <strong>in</strong> condensed-matter physics.<br />

7.1.3 The Helium atom<br />

The solution of Hartree-Fock equations <strong>in</strong> atoms also commonly uses the central<br />

field approximation. This allows to factorize Eqs.(7.11) <strong>in</strong>to a ra<strong>di</strong>al and<br />

an angular part, and to classify the solution with the ”tra<strong>di</strong>tional” quantum<br />

numbers n, l, m.<br />

For He, the Hartree-Fock equations, Eq.(7.11), reduce to<br />

∫<br />

− ¯h2 ∇ 2<br />

2m<br />

1φ 1 (1) − Zq2 e<br />

φ 1 (1) +<br />

e r 1<br />

∫<br />

+<br />

φ ∗ 1(2) q2 e<br />

r 12<br />

[φ 1 (2)φ 1 (1) − φ 1 (2)φ 1 (1)] dv 2<br />

φ ∗ 2(2) q2 e<br />

r 12<br />

[φ 2 (2)φ 1 (1) − δ(σ 1 , σ 2 )φ 1 (2)φ 2 (1)] dv 2 = ɛ 1 φ 1 (1) (7.19)<br />

S<strong>in</strong>ce the <strong>in</strong>tegrand <strong>in</strong> the first <strong>in</strong>tegral is zero,<br />

∫<br />

− ¯h2 ∇ 2<br />

2m<br />

1φ 1 (1) − Zq2 e<br />

φ 1 (1) + φ ∗<br />

e r<br />

2(2) q2 e<br />

[φ 2 (2)φ 1 (1)<br />

1 r 12<br />

−δ(σ 1 , σ 2 )φ 1 (2)φ 2 (1)] dv 2 = ɛ 1 φ 1 (1). (7.20)<br />

In the ground state, the two electrons have opposite sp<strong>in</strong> (δ(σ 1 , σ 2 ) = 0) and<br />

occupy the same spherically symmetric orbital (that is: φ 1 and φ 2 are the same<br />

function, φ). This means that the Hartree-Fock equation, Eq.(7.20), for the<br />

ground state is the same as the Hartree equation, Eq.(6.19). In fact, the two<br />

electrons have opposite sp<strong>in</strong> and there is thus no exchange.<br />

In general, one speaks of Restricted Hartree-Fock (RHF) for the frequent<br />

case <strong>in</strong> which all orbitals are present <strong>in</strong> pairs, formed by a same function of r,<br />

multiplied by sp<strong>in</strong> functions of opposite sp<strong>in</strong>. In the follow<strong>in</strong>g, this will always<br />

be the case.<br />

7.2 Code: helium hf gauss<br />

The ra<strong>di</strong>al solution of Hartree-Fock equations is possible only for atoms or <strong>in</strong><br />

some model systems. In most cases the solution is found by expand<strong>in</strong>g on a<br />

suitable basis set, <strong>in</strong> analogy with the variational method.<br />

Let us re-write the Hartree-Fock equation – for the restricted case, i.e. no<br />

total sp<strong>in</strong> – <strong>in</strong> the follow<strong>in</strong>g form:<br />

Fφ k = ɛ k φ k , k = 1, . . . , N/2 (7.21)<br />

The <strong>in</strong>dex k labels the coord<strong>in</strong>ate parts of the orbitals; for each k there is<br />

a sp<strong>in</strong>-up and a sp<strong>in</strong>-down orbital. F is called the Fock operator. It is of<br />

57

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